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Fig. 9


Azimuthally averaged surface brightness brightness profiles of the ε Eri dust disk (case “A”) at three Spitzer/MIPS wavelengths: 24   μm (top), 70   μm (middle), and 160   μm (bottom). Points with error bars: star-subtracted MIPS data (Fig. 6 of Backman et al. 2009). Solid lines: modeled profiles after convolution with the PSFs. Thin solid lines: the instrumental PSF.

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